RNAFOLD

NAME

SYNOPSIS

DESCRIPTION

It also produces PostScript files with plots of the resulting secondary structure graph and a "dot plot" of the base pairing matrix. The dot plot shows a matrix of squares with area proportional to the pairing probability in the upper right half, and one square for each pair in the minimum free energy structure in the lower left half. For each pair i-j with probability p>10E-6 there is a line of the form
i j sqrt(p) ubox
in the PostScript file, so that the pair probabilities can be easily extracted.

Sequences are read in a simple text format where each sequence occupies a single line. Each sequence may be preceded by a line of the form
> name
to assign a name to the sequence. If a name is given in the input
 PostScript files "name_ss.ps" and "name_dp.ps" are produced for the structure and dot plot, respectively. Otherwise the file names default to rna.ps and dot.ps. Existing files of the same name will be overwritten.
The input format is similar to fasta except that even long sequences may not be interrupted by line breaks, and the header lines are optional. The program will continue to read new sequences until a line consisting of the single character @ or an end of file condition is encountered.

OPTIONS

-p

Calculate the partition function and base pairing probability matrix in addition to the mfe structure. Default is calculation of mfe structure only. In addition to the MFE structure we print a coarse representation of the pair probabilities in form of a pseudo bracket notation, followed by the ensemble free energy, as well as the centroid structure derived from the pair probabilities together with its free energy and distance to the ensemble. Finally it prints the frequency of the mfe structure, and the structural diversity (mean distance between the structures in the ensemble). See the description of pf_fold() and mean_bp_dist() and centroid() in the RNAlib documentation for details.
Note that unless you also specify -d2 or -d0, the partition function and mfe calculations will use a slightly different energy model. See the discussion of dangling end options below.

-p0

Calculate the partition function but not the pair probabilities, saving about 50% in runtime. Prints the ensemble free energy -kT ln(Z).

-p2

In addition to pair probabilities compute stack probabilities, i.e. the probability that a pair (i,j) and the immediately interior pair (i+1,j-1) are formed simultaneously. A second postscript dot plot called "name_dp2.ps", or "dot2.ps" (if the sequence does not have a name), is produced that contains pair probabilities in the upper right half and stack probabilities in the lower left.

-C

Calculate structures subject to constraints. The program reads first the sequence, then a string containing constraints on the structure encoded with the symbols: | (the corresponding base has to be paired x (the base is unpaired) < (base i is paired with a base j>i) > (base i is paired with a base j<i) and matching brackets ( ) (base i pairs base j) With the exception of "|", constraints will disallow all pairs conflicting with the constraint. This is usually sufficient to enforce the constraint, but occasionally a base may stay unpaired in spite of constraints. PF folding ignores constraints of type "|".

-T temp

Rescale energy parameters to a temperature of temp C. Default is 37C.

-4

Do not include special stabilizing energies for certain tetra-loops. Mostly for testing.

-d[0|1|2|3]

How to treat "dangling end" energies for bases adjacent to helices in free ends and multi-loops: With (-d1) only unpaired bases can participate in at most one dangling end, this is the default for mfe folding but unsupported for the partition function folding. With -d2 this check is ignored, dangling energies will be added for the bases adjacent to a helix on both sides in any case; this is the default for partition function folding (-p). -d or -d0 ignores dangling ends altogether (mostly for debugging).
With -d3 mfe folding will allow coaxial stacking of adjacent helices in multi-loops. At the moment the implementation will not allow coaxial stacking of the two interior pairs in a loop of degree 3 and works only for mfe folding.
Note that by default (as well as with -d1 and -d3) pf and mfe folding treat dangling ends differently. Use -d2 in addition to -p to ensure that both algorithms use the same energy model.

-noLP

Produce structures without lonely pairs (helices of length 1). For partition function folding this only disallows pairs that can only occur isolated. Other pairs may still occasionally occur as helices of length 1.

-noGU

Do not allow GU pairs.

-noCloseGU

Do not allow GU pairs at the end of helices.

-e 1|2

Rarely used option to fold sequences from the artificial ABCD... alphabet, where A pairs B, C-D etc. Use the energy parameters for GC (-e 1) or AU (-e 2) pairs.

-P <paramfile>

Read energy parameters from paramfile, instead of using the default parameter set. A sample parameter file should accompany your distribution. See the RNAlib documentation for details on the file format.

-nsp pairs

Allow other pairs in addition to the usual AU,GC,and GU pairs. pairs is a comma separated list of additionally allowed pairs. If a the first character is a "-" then AB will imply that AB and BA are allowed pairs. e.g. RNAfold -nsp -GA will allow GA and AG pairs. Nonstandard pairs are given 0 stacking energy.

-S scale

In the calculation of the pf use scale*mfe as an estimate for the ensemble free energy (used to avoid overflows). The default is 1.07, useful values are 1.0 to 1.2. Occasionally needed for long sequences. You can also recompile the program to use double precision (see the README file).

-circ

Assume a circular (instead of linear) RNA molecule.

-noPS

Do not produce postscript drawing of the mfe structure.

REFERENCES

If you use this program in your work you might want to cite:

I.L. Hofacker, W. Fontana, P.F. Stadler, S. Bonhoeffer, M. Tacker, P. Schuster (1994) Fast Folding and Comparison of RNA Secondary Structures. Monatshefte f. Chemie 125: 167-188
M. Zuker, P. Stiegler (1981) Optimal computer folding of large RNA sequences using thermodynamic and auxiliary information, Nucl Acid Res 9: 133-148
J.S. McCaskill (1990) The equilibrium partition function and base pair binding probabilities for RNA secondary structures, Biopolymers 29: 1105-1119
I.L. Hofacker & P.F. Stadler (2006) Memory Efficient Folding Algorithms for Circular RNA Secondary Structures, Bioinformatics (2006)
A.F. Bompfünewerer, R. Backofen, S.H. Bernhart, J. Hertel, I.L. Hofacker, P.F. Stadler, S. Will (2007) "Variations on {RNA} Folding and Alignment: Lessons from Benasque" J. Math. Biol.
D. Adams (1979) The hitchhiker's guide to the galaxy, Pan Books, London

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